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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof Steven Balbus FRS, FInstP

Emeritus Savilian Professor

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Pulsars, transients and relativistic astrophysics
  • Theoretical astrophysics and plasma physics at RPC
steven.balbus@physics.ox.ac.uk
  • About
  • Publications

An exact, three-dimensional, time-dependent wave solution in local keplerian flow

Astrophysical Journal 652:2 I (2006) 1020-1027

Authors:

SA Balbus, JF Hawley

Abstract:

We present an exact three-dimensional wave solution to the shearing-sheet equations of motion. The existence of this solution argues against transient amplification as a route to turbulence in unmagnetized disks. Moreover, because the solution covers an extensive dynamical range in wavenumber space, it is an excellent test of the dissipative properties of numerical codes. 漏 2006. The American Astronomical Society. All rights reserved.

An exact, three-dimensional, time-dependent wave solution in local Keplerian flow

ASTROPHYSICAL JOURNAL 652:2 (2006) 1020-1027

Authors:

Steven A Balbus, John F Hawley

Fluid dynamics - Spinning discs in the lab

NATURE 444:7117 (2006) 281-+

Dynamics of the Magnetoviscous Instability

The Astrophysical Journal American Astronomical Society 633:1 (2005) 328-333

Authors:

Tanim Islam, Steven Balbus

Numerical Simulations of the MRI and real disks

Astrophysics of Cataclysmic Variables and Related Objects 330 (2005) 185-196

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